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Results 1 - 16 of 16
A distinct halo population revealed from 3D non-LTE magnesium abundances
Volume 19, Issue 21 - article #2
T. Matsuno
,
A. M. Amarsi
,
M. Carlos
,
P. E. Nissen
https://arxiv.org/abs/2405.13486
Raising the observed metallicity floor with a 3D non-LTE analysis of SDSS J102915.14+172927.9★
Volume 18, Issue 14 - article #5
C. Lagae
,
A. M. Amarsi
,
L. F. RodrÃguez DÃaz
,
K. Lind
,
T. Nordlander
,
T. T. Hansen
,
A. Heger
Astronomy & Astrophysics
https://www.aanda.org/10.1051/0004-6361/202245786
3D non-LTE iron abundances in FG-type dwarfs
Volume 17, Issue 48 - article #8
A. M. Amarsi
,
S. Liljegren
,
P. E. Nissen
Astronomy & Astrophysics
https://www.aanda.org/10.1051/0004-6361/202244542
3D non-LTE iron abundances in FG-type dwarfs. (arXiv:2209.13449v1 [astro-ph.SR])
Volume 17, Issue 38 - article #1
A. M. Amarsi
,
S. Liljegren
,
P. E. Nissen
http://arxiv.org/abs/2209.13449
The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines. (arXiv:2109.04752v1 [astro-ph.SR])
Volume 16, Issue 38 - article #7
A. M. Amarsi
,
N. Grevesse
,
M. Asplund
,
R. Collet
http://arxiv.org/abs/2109.04752
The GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys. (arXiv:2008.09582v1 [astro-ph.SR])
Volume 15, Issue 35 - article #8
A. M. Amarsi
,
K. Lind
,
Y. Osorio
,
T. Nordlander
,
M. Bergemann
,
H. Reggiani
,
E. X. Wang
,
S. Buder
,
M. Asplund
,
P. S. Barklem
,
A. Wehrhahn
,
Á. Skúladóttir
,
C. Kobayashi
,
A. I. Karakas
,
X. D. Gao
,
J. Bland-Hawthorn
,
G. M. De Silva
,
J. Kos
,
G. F. Lewis
,
S. L. Martell
,
S. Sharma
,
J. D. Simpson
,
D. B. Zucker
,
K. Čotar
,
J. Horner
,
the GALAH collaboration
http://arxiv.org/abs/2008.09582
The 3D non-LTE solar nitrogen abundance from atomic lines
Volume 15, Issue 18 - article #10
A. M. Amarsi
,
N. Grevesse
,
J. Grumer
,
M. Asplund
,
P. S. Barklem
,
R. Collet
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/niJ9_nZbpjE/202037890
The 3D non-LTE solar nitrogen abundance from atomic lines. (arXiv:2003.12561v1 [astro-ph.SR])
Volume 15, Issue 14 - article #3
A. M. Amarsi
,
N. Grevesse
,
J. Grumer
,
M. Asplund
,
P. S. Barklem
,
R. Collet
http://arxiv.org/abs/2003.12561
Carbon, oxygen, and iron abundances in disk and halo stars
Volume 14, Issue 39 - article #11
A. M. Amarsi
,
P. E. Nissen
,
Ã. Skúladóttir
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/DwS5xVkIfCA/201936265
3D non-LTE line formation of neutral carbon in the Sun
Volume 14, Issue 16 - article #10
A. M. Amarsi
,
P. S. Barklem
,
R. Collet
,
N. Grevesse
,
M. Asplund
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/q-K2LUMIZts/201833603
Carbon and oxygen in metal-poor halo stars⋆
Volume 14, Issue 5 - article #2
A. M. Amarsi
,
P. E. Nissen
,
M. Asplund
,
K. Lind
,
P. S. Barklem
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/QTipYx6aF8Y/201834480
Carbon and oxygen in metal-poor halo stars. (arXiv:1901.03592v1 [astro-ph.SR])
Volume 14, Issue 3 - article #1
A. M. Amarsi
,
P. E. Nissen
,
M. Asplund
,
K. Lind
,
P. S. Barklem
http://arxiv.org/abs/1901.03592
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
Volume 13, Issue 16 - article #12
S. Buder
(1,2),
M. Asplund
(3,4),
L. Duong
(3),
J. Kos
(5),
K. Lind
(1,6),
M. K. Ness
(7,8),
S. Sharma
(5,4),
J. Bland-Hawthorn
(5,4),
A. R. Casey
(9),
G. M. De Silva
(10,5),
V. D'Orazi
(11),
K. C. Freeman
(3),
G. F. Lewis
(5),
J. Lin
(3,4),
S. L. Martell
(12),
K. J. Schlesinger
(3),
J. D. Simpson
(10),
D. B. Zucker
(13,10),
T. Zwitter
(14),
A. M. Amarsi
(1),
B. Anguiano
(15),
D. Carollo
(16),
K. Cotar
(14),
P. L. Cottrell
(9,17),
G. Da Costa
(3),
X. D. Gao
(1),
M. R. Hayden
(5,4),
J. Horner
(18),
M. J. Ireland
(3),
P. R. Kafle
(19),
U. Munari
(20),
D. M. Nataf
(21),
T. Nordlander
(3,4),
Dennis Stello
(12,22,4),
Y.-S. Ting
(23,24,25),
G. Traven
(14),
F. Watson
(10,26),
R. A. Wittenmyer
(18),
R. F. G. Wyse
(21),
D. Yong
(3),
J. C. Zinn
(27),
M. Zerjal
(3)
((1) MPIA Heidelberg,
(2) IMPRS HD,
(3) RSAA/MSO Canberra,
(4) ASTRO-3D Australia,
(5) SIfA Sydney,
(6) Uppsala University,
(7) Columbia University New York,
(8) CCA New York
(9) Monash University,
(10) AAO North Ryde,
(11) INAF Padova,
(12) UNSW Sydney,
(13) Macquarie University Sydney,
(14) University of Ljubljana,
(15) University of Virginia,
(16) INAF Turin,
(17) University of Canterbury,
(18) University of Southern Queensland,
(19) University of Western Australia,
(20) INAF Padova,
(21) Johns Hopkins University Baltimore,
(22) Aarhus University,
(23) IAS Princeton,
(24) Princeton University,
(25) Carnegie Observatories Pasadena,
(26) Western Sydney University,
(27) The Ohio State University)
http://arxiv.org/abs/1804.06041
Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation. (arXiv:1804.02305v1 [astro-ph.SR])
Volume 13, Issue 15 - article #6
A. M. Amarsi
,
T. Nordlander
,
P. S. Barklem
,
M. Asplund
,
R. Collet
,
K. Lind
http://arxiv.org/abs/1804.02305
The Galactic chemical evolution of oxygen inferred from 3D non-LTE spectral line formation calculations
Volume 10, Issue 30 - article #13
A. M. Amarsi
,
M. Asplund
,
R. Collet
,
J. Leenaarts
arXiv.org - Astrophysics - Volume: 2015, Issue: 21 Aug
arXiv:1508.04857
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On line contribution functions and examining spectral line formation in 3D model stellar atmospheres
Volume 10, Issue 28 - article #10
A. M. Amarsi
Monthly Notices of the Royal Astronomical Society - Volume: 452, Issue: 2
Abstract
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